HARDY
发表于 2025-3-21 16:34:31
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效果
发表于 2025-3-21 21:51:36
0067-0057of communication between theoreticians and observers and between different schools of thought, in spite of the advances of recent years in certain directions (observations of ordinary novae at minimum and of dwarf novae, theory of the causes of the explosion, etc ••• ). The meeting whose proceeding
instulate
发表于 2025-3-22 01:15:23
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可忽略
发表于 2025-3-22 06:59:12
Physical Parameters of Prenovae and Outburst Amplitudesres and white dwarf densities are, however, mutually exclusive over a wide range of M.. Only two novae, CP Pup and V1500 Cyg, have, under the assumption of O-type temperatures, densities within the white dwarf range and even they are found near the low-density limit. This leaves three explanations for minimum light:
fledged
发表于 2025-3-22 12:33:00
Past and Future Novaes (NZ,), and dwarf novae, including U Geminorum stars (UG) and Z Camelopardalis stars (Z Cam). We exclude supernovae from the present discussion, and summarize the content and interrelationships of the other classes.
intention
发表于 2025-3-22 14:12:11
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抱怨
发表于 2025-3-22 20:46:26
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丛林
发表于 2025-3-22 23:34:53
The Expansion of Novae before Light Maximum and the Formation of the Principal Envelopeed from the moment of explosion of a Nova up to the moment of appearance of the principal spectrum of the star. At first we should mention that already for three Novae we have information on their spectra, obtained before the explosion by means of objective prisms, see discussion of this in paper of Arhipova and Mustel (1975).
Meager
发表于 2025-3-23 02:12:25
The Binary Nature of the Nova-Like Variable CD -42° 14462 velocity and intensity of these emissions indicates a hot spot on the following side of the accretion disk. Simultaneous rapid photometry reveals the flickering is not modulated with the orbital period, suggesting the inclination is too low for an eclipse or occultation of the hot spot.
净礼
发表于 2025-3-23 06:08:17
Model of Nova Envelopesculations (Starrfield, Sparks, and Truran 1974), and by an analytical study (Nariai 1974). The latter predicts the increase in Te and almost constant L for the quasi-static envelope for a period of 0.5 . where ..